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Explanation: Reflection nebulas reflect light from a nearby star. Many small carbon grains in the nebula reflect the light. The blue color typical of reflection nebula is caused by blue light being more efficiently scattered by the carbon dust than red light. The brightness of the nebula is determined by the size and density of the reflecting grains, and by the color and brightness of the neighboring star(s). NGC 1435, pictured above, surrounds Merope (23 Tau), one of the brightest stars in the Pleiades (M45). The Pleiades nebulosity is caused by a chance encounter between an open cluster of stars and a molecular cloud.
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: reflection nebula - Merope
Publications with words: reflection nebula - Merope
See also:
- APOD: 2026 April 7 Á IC 4592: The Blue Horsehead Reflection Nebula
- APOD: 2026 February 2 Á Orion: The Running Man Nebula
- NGC 1333: Stellar Nursery in Perseus
- APOD: 2026 January 28 Á M78: Reflecting Blue in a Sea of Red
- NGC 7023: The Iris Nebula
- APOD: 2025 September 19 Á The NGC 6914 Complex
- Reflections on VdB 31